Galaxy groups are more than an intermediate scale between clusters and halos hosting
individual galaxies, they are crucial laboratories capable of testing a range of astrophysics …

Contrary to many stereotypes about massive galaxies, observed brightest group galaxies
(BGGs) are diverse in their star formation rates, kinematic properties, and morphologies …

We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

The early release science results from JWST have yielded an unexpected abundance of
high-redshift luminous galaxies that seems to be in tension with current theories of galaxy …

We present an analysis of the quenching of star formation in galaxies, bulges, and disks
throughout the bulk of cosmic history, from z= 2− 0. We utilise observations from the Sloan …

Understanding the variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

We compare the star-forming main sequence (SFMS) of galaxies–both integrated and
resolved on 1 kpc scales–between the high-resolution TNG50 simulation of IllustrisTNG and …

There has been a long-standing factor-of-two tension between the observed star formation
rate density and the observed stellar mass buildup after z∼ 2. Recently, we have proposed …

We use the TNG100 simulation of the IllustrisTNG project to investigate the stellar specific
angular momenta (j*) of∼ 12 000 central galaxies at z= 0 in a full cosmological context, with …

We present a catalog of about 25,000 images of massive (M⋆≥ 10 9 M⊙) galaxies at
redshifts 3≤ z≤ 6 from the TNG50 cosmological simulation, tailored for observations at …